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Sabbatical Leave Report 2019 – 2020
Sabbatical Leave Report 2019 – 2020 James MacDevitt, M.A. Associate Professor of Art History and Visual & Cultural Studies Director, Cerritos College Art Gallery Department of Art and Design Fine Arts and Communications Division Cerritos College January 2021 Table of Contents Title Page i Table of Contents ii Sabbatical Leave Application iii Statement of Purpose 35 Objectives and Outcomes 36 OER Textbook: Disciplinary Entanglements 36 Getty PST Art x Science x LA Research Grant Application 37 Conference Presentation: Just Futures 38 Academic Publication: Algorithmic Culture 38 Service and Practical Application 39 Concluding Statement 40 Appendix List (A-E) 41 A. Disciplinary Entanglements | Table of Contents 42 B. Disciplinary Entanglements | Screenshots 70 C. Getty PST Art x Science x LA | Research Grant Application 78 D. Algorithmic Culture | Book and Chapter Details 101 E. Just Futures | Conference and Presentation Details 103 2 SABBATICAL LEAVE APPLICATION TO: Dr. Rick Miranda, Jr., Vice President of Academic Affairs FROM: James MacDevitt, Associate Professor of Visual & Cultural Studies DATE: October 30, 2018 SUBJECT: Request for Sabbatical Leave for the 2019-20 School Year I. REQUEST FOR SABBATICAL LEAVE. I am requesting a 100% sabbatical leave for the 2019-2020 academic year. Employed as a fulltime faculty member at Cerritos College since August 2005, I have never requested sabbatical leave during the past thirteen years of service. II. PURPOSE OF LEAVE Scientific advancements and technological capabilities, most notably within the last few decades, have evolved at ever-accelerating rates. Artists, like everyone else, now live in a contemporary world completely restructured by recent phenomena such as satellite imagery, augmented reality, digital surveillance, mass extinctions, artificial intelligence, prosthetic limbs, climate change, big data, genetic modification, drone warfare, biometrics, computer viruses, and social media (and that’s by no means meant to be an all-inclusive list). -
UNITED STATES DISTRICT COURT NORTHERN DISTRICT of INDIANA SOUTH BEND DIVISION in Re FEDEX GROUND PACKAGE SYSTEM, INC., EMPLOYMEN
USDC IN/ND case 3:05-md-00527-RLM-MGG document 3279 filed 03/22/19 page 1 of 354 UNITED STATES DISTRICT COURT NORTHERN DISTRICT OF INDIANA SOUTH BEND DIVISION ) Case No. 3:05-MD-527 RLM In re FEDEX GROUND PACKAGE ) (MDL 1700) SYSTEM, INC., EMPLOYMENT ) PRACTICES LITIGATION ) ) ) THIS DOCUMENT RELATES TO: ) ) Carlene Craig, et. al. v. FedEx Case No. 3:05-cv-530 RLM ) Ground Package Systems, Inc., ) ) PROPOSED FINAL APPROVAL ORDER This matter came before the Court for hearing on March 11, 2019, to consider final approval of the proposed ERISA Class Action Settlement reached by and between Plaintiffs Leo Rittenhouse, Jeff Bramlage, Lawrence Liable, Kent Whistler, Mike Moore, Keith Berry, Matthew Cook, Heidi Law, Sylvia O’Brien, Neal Bergkamp, and Dominic Lupo1 (collectively, “the Named Plaintiffs”), on behalf of themselves and the Certified Class, and Defendant FedEx Ground Package System, Inc. (“FXG”) (collectively, “the Parties”), the terms of which Settlement are set forth in the Class Action Settlement Agreement (the “Settlement Agreement”) attached as Exhibit A to the Joint Declaration of Co-Lead Counsel in support of Preliminary Approval of the Kansas Class Action 1 Carlene Craig withdrew as a Named Plaintiff on November 29, 2006. See MDL Doc. No. 409. Named Plaintiffs Ronald Perry and Alan Pacheco are not movants for final approval and filed an objection [MDL Doc. Nos. 3251/3261]. USDC IN/ND case 3:05-md-00527-RLM-MGG document 3279 filed 03/22/19 page 2 of 354 Settlement [MDL Doc. No. 3154-1]. Also before the Court is ERISA Plaintiffs’ Unopposed Motion for Attorney’s Fees and for Payment of Service Awards to the Named Plaintiffs, filed with the Court on October 19, 2018 [MDL Doc. -
Production and Saturation of Porosity in the Lunar Highlands from Impact Cratering
The fractured Moon: Production and saturation of porosity in the lunar highlands from impact cratering The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Soderblom, Jason M., et al. “The Fractured Moon: Production and Saturation of Porosity in the Lunar Highlands from Impact Cratering.” Geophysical Research Letters, vol. 42, no. 17, Sept. 2015, pp. 6939–44. © 2015 American Geophysical Union As Published http://dx.doi.org/10.1002/2015GL065022 Publisher American Geophysical Union (AGU) Version Final published version Citable link http://hdl.handle.net/1721.1/118615 Terms of Use Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. PUBLICATIONS Geophysical Research Letters RESEARCH LETTER The fractured Moon: Production and saturation 10.1002/2015GL065022 of porosity in the lunar highlands Key Points: from impact cratering • The relation between impact-generated porosity and crater size is quantified Jason M. Soderblom1, Alexander J. Evans2, Brandon C. Johnson1, H. Jay Melosh3, Katarina Miljković1,4, • Impacts into highly porous targets 5 6 7 8 3 result in positive gravity anomalies Roger J. Phillips , Jeffrey C. Andrews-Hanna , Carver J. Bierson , James W. Head III , Colleen Milbury , 9 7 1 2,10 11 • The cratering record of the oldest Gregory A. Neumann , Francis Nimmo , David E. Smith , Sean C. Solomon , Michael M. Sori , lunar surfaces is preserved in the -
An Impacting Descent Probe for Europa and the Other Galilean Moons of Jupiter
An Impacting Descent Probe for Europa and the other Galilean Moons of Jupiter P. Wurz1,*, D. Lasi1, N. Thomas1, D. Piazza1, A. Galli1, M. Jutzi1, S. Barabash2, M. Wieser2, W. Magnes3, H. Lammer3, U. Auster4, L.I. Gurvits5,6, and W. Hajdas7 1) Physikalisches Institut, University of Bern, Bern, Switzerland, 2) Swedish Institute of Space Physics, Kiruna, Sweden, 3) Space Research Institute, Austrian Academy of Sciences, Graz, Austria, 4) Institut f. Geophysik u. Extraterrestrische Physik, Technische Universität, Braunschweig, Germany, 5) Joint Institute for VLBI ERIC, Dwingelo, The Netherlands, 6) Department of Astrodynamics and Space Missions, Delft University of Technology, The Netherlands 7) Paul Scherrer Institute, Villigen, Switzerland. *) Corresponding author, [email protected], Tel.: +41 31 631 44 26, FAX: +41 31 631 44 05 1 Abstract We present a study of an impacting descent probe that increases the science return of spacecraft orbiting or passing an atmosphere-less planetary bodies of the solar system, such as the Galilean moons of Jupiter. The descent probe is a carry-on small spacecraft (< 100 kg), to be deployed by the mother spacecraft, that brings itself onto a collisional trajectory with the targeted planetary body in a simple manner. A possible science payload includes instruments for surface imaging, characterisation of the neutral exosphere, and magnetic field and plasma measurement near the target body down to very low-altitudes (~1 km), during the probe’s fast (~km/s) descent to the surface until impact. The science goals and the concept of operation are discussed with particular reference to Europa, including options for flying through water plumes and after-impact retrieval of very-low altitude science data. -
James A. Sinclair
James A. Sinclair MS 183-601, Jet Propulsion Laboratory Research Scientist 4800 Oak Grove Dr, Pasadena, CA 91109 Jet Propulsion Laboratory/Caltech E-mail: [email protected] Tel: +1 (818) 354-4853 Education 2010 - 2014 DPhil Atmospheric, Oceanic & Planetary Physics, University of Oxford, Oxford, United Kingdom. Thesis title: “Seasonal and interannual variability in Saturn’s stratosphere” Advisor: Prof. Patrick Irwin 2006 - 2010 MPhys Astrophysics (1st class), University of St. Andrews, St. Andrews, United Kingdom Thesis title: “Impact of stellar model spectra on disc detection” Advisor: Dr. Christiane Helling Research Experience 2018-Present Research Scientist, Jet Propulsion Laboratory/Caltech, Pasadena, CA, United States. • Auroral forcing of Jupiter’s stratospheric thermal structure and chemistry from mid-infrared spectroscopy. • Mid-infrared measurements and analysis of Jupiter’s dynamic weather layer to support the Juno mission. • Non-LTE radiative-transfer modelling of Jupiter’s atmosphere. • Seasonal variability in Saturn’s atmosphere. • Coupling of Neptune’s troposphere and stratosphere. • Influence of comet/asteroid impacts on Jupiter’s atmosphere. • Science collaborator for development of next-generation planetary-science instruments. 2015-2018 NASA Postdoctoral Fellow, Jet Propulsion Laboratory/Caltech, Pasadena, CA, United States Mentor: Dr. Glenn Orton • Auroral forcing of Jupiter’s stratospheric thermal structure and chemistry from mid-infrared spectroscopy. • Mid-infrared measurements and analysis of Jupiter’s dynamic weather layer to support the Juno mission. • Retrieval analyses of Voyager and Cassini spectra to derive atmospheric information at Jupiter’s poles. 2014-2015 Postdoctoral Research Assistant, Atmospheric, Oceanic & Planetary Physics, University of Oxford, Oxford, United Kingdom. Supervisors: Prof. Patrick Irwin, Dr. Simon Calcutt • Forward-model spectra simulations of the Martian atmosphere in nadir, limb and occultation sounding. -
Regional Oral History Off Ice University of California the Bancroft Library Berkeley, California
Regional Oral History Off ice University of California The Bancroft Library Berkeley, California Richard B. Gump COMPOSER, ARTIST, AND PRESIDENT OF GUMP'S, SAN FRANCISCO An Interview Conducted by Suzanne B. Riess in 1987 Copyright @ 1989 by The Regents of the University of California Since 1954 the Regional Oral History Office has been interviewing leading participants in or well-placed witnesses to major events in the development of Northern California, the West,and the Nation. Oral history is a modern research technique involving an interviewee and an informed interviewer in spontaneous conversation. The taped record is transcribed, lightly edited for continuity and clarity, and reviewed by the interviewee. The resulting manuscript is typed in final form, indexed, bound with photographs and illustrative materials, and placed in The Bancroft Library at the University of California, Berkeley, and other research collections for scholarly use. Because it is primary material, oral history is not intended to present the final, verified, or complete narrative of events. It is a spoken account, offered by the interviewee in response to questioning, and as such it is reflective, partisan, deeply involved, and irreplaceable. All uses of this manuscript are covered by a legal agreement between the University of California and Richard B. Gump dated 7 March 1988. The manuscript is thereby made available for research purposes. All literary rights in the manuscript, including the right to publish, are reserved to The Bancroft Library of the University of California, Berkeley. No part of the manuscript may be quoted for publication without the written permission of the Director of The Bancroft Library of the University of California, Berkeley. -
PDS Mission Interface for Europa Mission Status of Planning for Data Archiving
PDS Mission Interface for Europa Mission Status of Planning for Data Archiving CARTOGRAPHY AND IMAGING SCIENCES (“Imaging”) NODE PDS Lead Node Lisa Gaddis (USGS, Astrogeology) August 2016 Overview Common goals PDS4 Archiving roles, responsibilities EM archiving deliverables Data and Archive Working Group (DAWG) Archiving assignments Archiving activities to date Archiving schedule Current archiving activities Where we are now August 2016 2 Common Goals The PDS and Europa Mission (EM) will work together to ensure that we Organize, document and format EM digital planetary data in a standardized manner Collect complete, well-documented, peer-reviewed planetary data into archives Make planetary data available and useful to the science community ○ Provide online data delivery tools & services Ensure the long-term preservation and usability of the data August 2016 3 PDS4 The new PDS, an integrated data system to improve access ○ Required for all missions (e.g., used by LADEE, MAVEN) A re-architected, modern, online data system ○ Data are organized into bundles Includes all data for a particular instrument (e.g., PDF/A documents) ○ Bundles have collections Grouped files with a similar origin (e.g., Document Collection) Improves efficiency of ingestion and distribution of data ○ Uses Extensible Markup Language (XML) and standard data format templates ○ Self-consistent information model & software system ○ Information for Data Providers https://pds.nasa.gov/pds4/about ○ PDS4 Concepts Document https://pds.nasa.gov/pds4/doc/concepts/Concepts_150909.pdf -
Using the Galileo Solid-State Imaging Instrument As a Sensor of Jovian
Using the Galileo Solid-State Imaging Instrument as a Sensor of Jovian Energetic Electrons Ashley Carlton1, Maria de Soria-Santacruz Pich2, Insoo Jun2, Wousik Kim2, and Kerri Cahoy1 1Massachusetts Institute of Technology, Cambridge, 02139, USA (e-mail: [email protected]) 2Jet Propulsion Laboratory, California Institute of Technology, Pasadena, 91109, USA respectively. For the most part, information about the Jovian I. INTRODUCTION environment comes from the Galileo spacecraft Energetic Harsh radiation in the form of ionized, highly energetic Particle Detector (EPD) [Williams et al., 1992] (in Jovian particles is part of the space environment and can affect orbit from December 1995 to September 2003), which had a spacecraft. These particles not only sweep through the solar nearly equatorial orbit. Juno, a NASA spacecraft that entered system in the solar wind and flares and are ejected from Jovian orbit in July 2016, and Europa Clipper, a NASA galactic and extra-galactic supernovae, but also are trapped as mission planned for the 2020s, do not carry instruments belts in planetary magnetic fields. Jupiter’s magnetosphere is capable of measuring high-energy (>1 MeV) electrons. Juno is the largest and strongest of a planet in the solar system. in a polar orbit; Europa Clipper is planned to be in a highly Similar to Earth, Jupiter is roughly a magnetic dipole with a elliptical Jovian orbit, flying-by Jupiter’s moon, Europa, in tilt of ~11° [Khurana et al., 2004]. Jupiter’s magnetic field each orbit. strength is an order of magnitude larger than Earth, and its We develop a technique to extract the high-energy magnetic moment is roughly 18,000 times larger [Bagenal et electron environment using scientific imager data. -
Montana Alumnus
The Montana Alumnus Official Quarterly of The Alumni Association of the Slate University of Montana TRIBUTE TO MONTANA FOOTBALL GLIMPSES NEW FACULTY ALUMNI ACTIVITIES UNIVERSITY NOTES CLASS NOTES Volume XI NO. 2 Published in October, January, April, and July at Missoula, Montana )o; ®1|? iflmttmta Alumnus Published in October, January, April, and July by the Alumni Association of the State University of Montana. Subscription: 75c a year; subscription and annual dues of the Alumni Association combined, $1.50 a year. Printed by the School of Journalism Press, State University of M ontana. Entered as second-class matter November 1, 1922, at the postoffice a t M issoula, M ontana, under the A ct of M arch 3, 1879. Jessie Treichler, '29, Editor. Henrietta Wilhelm, ’25* Editor of Class Notes. THE ALUMNI ASSOCIATION OF THE STATE UNIVERSITY OF MONTANA JO H N PA TTERSO N , '20 ............................................................................... President BU RTT R. SMITH, ’27....................................................................................... Vice-President E. K. BADGLEY, '24 ..................................... Secretary-Treasurer DELEGATES TO THE EXECUTIVE COMMITTEE OAKLEY E. C O FFEE, '23 .......................................................................................................... Three-Y ear Delegate ROGER FLEM IN G , '26 .................................................................................................................Three-Y ear Delegate GORDON D. ROGNLIEN, '30...................................................................... -
Redalyc.Búsqueda General Con La Cámara Mosaico CCD Del
Revista Mexicana de Física ISSN: 0035-001X [email protected] Sociedad Mexicana de Física A.C. México Ferrín, I.; Leal, C.; Hernandez, J. Búsqueda general con la cámara mosaico CCD del telescopio Schmidt de 1m del Observatorio Nacional de Venezuela Revista Mexicana de Física, vol. 52, núm. 3, mayo, 2006, pp. 9-11 Sociedad Mexicana de Física A.C. Distrito Federal, México Disponible en: http://www.redalyc.org/articulo.oa?id=57020393003 Cómo citar el artículo Número completo Sistema de Información Científica Más información del artículo Red de Revistas Científicas de América Latina, el Caribe, España y Portugal Página de la revista en redalyc.org Proyecto académico sin fines de lucro, desarrollado bajo la iniciativa de acceso abierto ASTROFISICA´ REVISTA MEXICANA DE FISICA´ S 52 (3) 9–11 MAYO 2006 Busqueda´ general con la camara´ mosaico CCD del telescopio Schmidt de 1m del Observatorio Nacional de Venezuela I. Ferr´ın y C. Leal Facultad de Ciencias, Departamento de F´ısica, Centro de Astrof´ısica Teorica,´ Universidad de Los Andes Merida,´ Venezuela J. Hernandez Centro de investigaciones de astronom´ıa, CIDA, Merida,´ Venezuela Recibido el 25 de noviembre de 2003; aceptado el 12 de octubre de 2004 En el presente trabajo se muestran los resultados del programa de busqueda´ y seguimiento de diversos objetos astronomicos:´ estrellas variables, supernovas y objetos en movimiento dentro del Sistema Solar. Para ello estamos utilizando el telescopio Schmidt de 1m de diametro´ del Observatorio Nacional de Venezuela, el cual tiene acoplado una camara´ mosaico CCD de 67 Megap´ıxeles, en un arreglo de 4 £ 4 CCDs, cada uno de 2048 £ 2048 p´ıxeles. -
Flynn Creek Crater, Tennessee: Final Report, by David J
1967010060 ASTROGEOLOGIC STUDIES / ANNUAL PROGRESS REPORT " July 1, 1965 to July 1, 1966 ° 'i t PART B - h . CRATERINVESTIGATIONS N 67_1_389 N 57-" .]9400 (ACCEC_ION [4U _" EiER! (THRU} .2_ / PP (PAGLS) (CO_ w ) _5 (NASA GR OR I"MX OR AD NUMBER) (_ATEGORY) DEPARTMENT OF THE INTERIOR UNITED STATES GEOLOQICAL SURVEY • iri i i i i iiii i i 1967010060-002 ASTROGEOLOGIC STUDIES ANNUAL PROGRESS REPORT July i, 1965 to July I, 1966 PART B: CRATER INVESTIGATIONS November 1966 This preliminary report is distributed without editorial and technical review for conformity with official standards and nomenclature. It should not be quoted without permission. This report concerns work done on behalf of the National Aeronautics and Space Administration. DEPARTMENT OF THE INTERIOR UNITED STATES GEOLOGICAL SURVEY 1967010060-003 • #' C OING PAGE ,BLANK NO/" FILMED. CONTENTS PART B--CRATER INVESTIGATIONS Page Introduction ........................ vii History and origin of the Flynn Creek crater, Tennessee: final report, by David J. Roddy .............. 1 Introductien ..................... 1 Geologic history of the Flynn Creek crater ....... 5 Origin of the Flynn Creek crater ............ ii Conc lusions ...................... 32 References cited .................... 35 Geology of the Sierra Madera structure, Texas: progress report, by H. G. Wilshire ............ 41_ Introduction ...................... 41 Stratigraphy ...................... 41 Petrography and chemical composition .......... 49 S truc ture ....................... 62 References cited ............. ...... 69 Some aspects of the Manicouagan Lake structure in Quebec, Canada, by Stephen H. Wolfe ................ 71 f Craters produced by missile impacts, by H. J. Moore ..... 79 Introduction ...................... 79 Experimental procedure ................. 80 Experimental results .................. 81 Summary ........................ 103 References cited .................... 103 Hypervelocity impact craters in pumice, by H. J. Moore and / F. -
Artificial Intelligence at the Jet Propulsion Laboratory
AI Magazine Volume 18 Number 1 (1997) (© AAAI) Articles Making an Impact Artificial Intelligence at the Jet Propulsion Laboratory Steve Chien, Dennis DeCoste, Richard Doyle, and Paul Stolorz ■ The National Aeronautics and Space Administra- described here is in the context of the remote- tion (NASA) is being challenged to perform more agent autonomy technology experiment that frequent and intensive space-exploration mis- will fly on the New Millennium Deep Space sions at greatly reduced cost. Nowhere is this One Mission in 1998 (a collaborative effort challenge more acute than among robotic plane- involving JPL and NASA Ames). Many of the tary exploration missions that the Jet Propulsion AI technologists who work at NASA expected Laboratory (JPL) conducts for NASA. This article describes recent and ongoing work on spacecraft to have the opportunity to build an intelli- autonomy and ground systems that builds on a gent spacecraft at some point in their careers; legacy of existing success at JPL applying AI tech- we are surprised and delighted that it has niques to challenging computational problems in come this early. planning and scheduling, real-time monitoring By the year 2000, we expect to demonstrate and control, scientific data analysis, and design NASA spacecraft possessing on-board automat- automation. ed goal-level closed-loop control in the plan- ning and scheduling of activities to achieve mission goals, maneuvering and pointing to execute these activities, and detecting and I research and technology development resolving of faults to continue the mission reached critical mass at the Jet Propul- without requiring ground support. At this Asion Laboratory (JPL) about five years point, mission accomplishment can begin to ago.